NEAR-INFRARED CIRCULAR AND LINEAR POLARIMETRY OF MONOCEROS R2

被引:9
|
作者
Kwon, Jungmi [1 ,2 ,3 ]
Tamura, Motohide [1 ,2 ,4 ]
Hough, James H. [5 ]
Nagata, Tetsuya [6 ]
Kusakabe, Nobuhiko [2 ]
机构
[1] Univ Tokyo, Dept Astron, Grad Sch Sci, Tokyo 1130033, Japan
[2] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[3] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
[4] Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
[5] Univ Hertfordshire, Hatfield AL10 9AB, Herts, England
[6] Kyoto Univ, Sakyo Ku, Kyoto 6068502, Japan
来源
ASTRONOMICAL JOURNAL | 2016年 / 152卷 / 03期
基金
新加坡国家研究基金会;
关键词
circumstellar matter; infrared: stars; ISM: individual objects (Mon R2); ISM: structure; polarization; stars: formation; YOUNG STELLAR OBJECTS; STAR-FORMING REGIONS; T-TAURI STARS; MON R2; IMAGING POLARIMETRY; POLARIZATION MAPS; MOLECULAR CLOUDS; HIGH-RESOLUTION; ORION-A; CORE;
D O I
10.3847/0004-6256/152/3/67
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have conducted simultaneous JHKs-band imaging circular and linear polarimetry of the Monoceros R2 (Mon R2) cluster. We present results from deep and wide near-infrared linear polarimetry of the Mon R2 region. Prominent and extended polarized nebulosities over the Mon R2 field are revisited, and an infrared reflection nebula associated with the Mon R2 cluster and two local reflection nebulae, vdB 67 and vdB 69, is detected. We also present results from deep imaging circular polarimetry in the same region. For the first time, the observations show relatively high degrees of circular polarization (CP) in Mon R2, with as much as approximately 10% in the K-s band. The maximum CP extent of a ring-like nebula around the Mon R2 cluster is approximately 0.60 pc, while that of a western nebula, around vdB 67, is approximately 0.24 pc. The extended size of the CP is larger than those seen in the Orion region around IRc2, while the maximum degree of CP of similar to 10% is smaller than those of similar to 17% seen in the Orion region. Nonetheless, both the CP size and degree of this region are among the largest in our infrared CP survey of star-forming regions. We have also investigated the time variability of the degree of the polarization of several infrared sources and found possible variations in three sources.
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页数:13
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